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UTC(LRTE) H-Maser maintenace

LP
Luiz Paulo Damaceno
Mon, May 25, 2026 6:38 PM

Hi all,

I've started to see if is possible to fix an H-maser that we have here in
our timelab. Today we're contributing to UTC With some ensemble that is
composed by: 1 commercial cs clock + BVA phase locked in long term (<100s)
to the cs + synthesizer + HROG-5. And these are results for last circular
t: Cirt 460 LRTE PPP link
https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb.333a_.gif
I
wish to know if this result is good for an ensemble like we  have here for
starting this discussion... And what you all suggest for improvement. Today
i have:

Real time tropospheric delay calculation with hopfield's model to replace
"MDTR" (with also mapping function to correct for each satellite). Every 15
minutes, also, I fed the Rx5Tr receiver with temperature, humidity and
pressure for its tropospheric model update. The sensor is located near the
antenna.

And an algorithm that simply sees the frequency deviation every 2 hours and
computes a frequency correction for our HROG-5.

We also have a hydrogen maser that is stopped because the 10 MHz oscillator
is not locking. I want to do some maintenance there to see if it can be
brought back to life.

The maser is glowing purple, but it shows "no vacuum" and "synthesizer is
faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the
cavity output, but nothing more.

So, if possible, I may want to be guided in some steps to see if is it
possible to recover it.

Best regards,

Luiz

Hi all, I've started to see if is possible to fix an H-maser that we have here in our timelab. Today we're contributing to UTC With some ensemble that is composed by: 1 commercial cs clock + BVA phase locked in long term (<100s) to the cs + synthesizer + HROG-5. And these are results for last circular t: Cirt 460 LRTE PPP link <https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb.333a_.gif> I wish to know if this result is good for an ensemble like we have here for starting this discussion... And what you all suggest for improvement. Today i have: Real time tropospheric delay calculation with hopfield's model to replace "MDTR" (with also mapping function to correct for each satellite). Every 15 minutes, also, I fed the Rx5Tr receiver with temperature, humidity and pressure for its tropospheric model update. The sensor is located near the antenna. And an algorithm that simply sees the frequency deviation every 2 hours and computes a frequency correction for our HROG-5. We also have a hydrogen maser that is stopped because the 10 MHz oscillator is not locking. I want to do some maintenance there to see if it can be brought back to life. The maser is glowing purple, but it shows "no vacuum" and "synthesizer is faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the cavity output, but nothing more. So, if possible, I may want to be guided in some steps to see if is it possible to recover it. Best regards, Luiz
J
john@miles.io
Tue, May 26, 2026 5:48 AM

The Cs+GNSS ensemble looks like it's performing very well.  That's the
Septentrio PolaRx5TR receiver, correct?

It sounds like you may have a power supply problem with the maser, or
perhaps a controller issue, since you obviously have vacuum if the
dissociator is lit.  How far off frequency is it?  More than a few Hz
suggests that the oscillator oven has failed, which could explain everything
except the vacuum error.

-- john

-----Original Message-----
From: Luiz Paulo Damaceno via time-nuts time-nuts@lists.febo.com
Sent: Monday, May 25, 2026 11:39 AM
To: Discussion of precise time and frequency measurement
time-nuts@lists.febo.com
Cc: Luiz Paulo Damaceno luizpauloeletrico42@gmail.com
Subject: [time-nuts] UTC(LRTE) H-Maser maintenace

Hi all,

I've started to see if is possible to fix an H-maser that we have here in
our timelab. Today we're contributing to UTC With some ensemble that is
composed by: 1 commercial cs clock + BVA phase locked in long term (<100s)
to the cs + synthesizer + HROG-5. And these are results for last circular
t: Cirt 460 LRTE PPP link
<https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb.
333a_.gif>
I
wish to know if this result is good for an ensemble like we  have here for
starting this discussion... And what you all suggest for improvement. Today
i have:

Real time tropospheric delay calculation with hopfield's model to replace
"MDTR" (with also mapping function to correct for each satellite). Every 15
minutes, also, I fed the Rx5Tr receiver with temperature, humidity and
pressure for its tropospheric model update. The sensor is located near the
antenna.

And an algorithm that simply sees the frequency deviation every 2 hours and
computes a frequency correction for our HROG-5.

We also have a hydrogen maser that is stopped because the 10 MHz oscillator
is not locking. I want to do some maintenance there to see if it can be
brought back to life.

The maser is glowing purple, but it shows "no vacuum" and "synthesizer is
faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the
cavity output, but nothing more.

So, if possible, I may want to be guided in some steps to see if is it
possible to recover it.

Best regards,

Luiz


time-nuts mailing list -- time-nuts@lists.febo.com To unsubscribe send an
email to time-nuts-leave@lists.febo.com

The Cs+GNSS ensemble looks like it's performing very well. That's the Septentrio PolaRx5TR receiver, correct? It sounds like you may have a power supply problem with the maser, or perhaps a controller issue, since you obviously have vacuum if the dissociator is lit. How far off frequency is it? More than a few Hz suggests that the oscillator oven has failed, which could explain everything except the vacuum error. -- john -----Original Message----- From: Luiz Paulo Damaceno via time-nuts <time-nuts@lists.febo.com> Sent: Monday, May 25, 2026 11:39 AM To: Discussion of precise time and frequency measurement <time-nuts@lists.febo.com> Cc: Luiz Paulo Damaceno <luizpauloeletrico42@gmail.com> Subject: [time-nuts] UTC(LRTE) H-Maser maintenace Hi all, I've started to see if is possible to fix an H-maser that we have here in our timelab. Today we're contributing to UTC With some ensemble that is composed by: 1 commercial cs clock + BVA phase locked in long term (<100s) to the cs + synthesizer + HROG-5. And these are results for last circular t: Cirt 460 LRTE PPP link <https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb. 333a_.gif> I wish to know if this result is good for an ensemble like we have here for starting this discussion... And what you all suggest for improvement. Today i have: Real time tropospheric delay calculation with hopfield's model to replace "MDTR" (with also mapping function to correct for each satellite). Every 15 minutes, also, I fed the Rx5Tr receiver with temperature, humidity and pressure for its tropospheric model update. The sensor is located near the antenna. And an algorithm that simply sees the frequency deviation every 2 hours and computes a frequency correction for our HROG-5. We also have a hydrogen maser that is stopped because the 10 MHz oscillator is not locking. I want to do some maintenance there to see if it can be brought back to life. The maser is glowing purple, but it shows "no vacuum" and "synthesizer is faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the cavity output, but nothing more. So, if possible, I may want to be guided in some steps to see if is it possible to recover it. Best regards, Luiz _______________________________________________ time-nuts mailing list -- time-nuts@lists.febo.com To unsubscribe send an email to time-nuts-leave@lists.febo.com
AK
Attila Kinali
Tue, May 26, 2026 6:04 AM

A wonderful good morning!

On Mon, 25 May 2026 15:38:54 -0300
Luiz Paulo Damaceno via time-nuts time-nuts@lists.febo.com wrote:

I've started to see if is possible to fix an H-maser that we have here in
our timelab. Today we're contributing to UTC With some ensemble that is
composed by: 1 commercial cs clock + BVA phase locked in long term (<100s)
to the cs + synthesizer + HROG-5. And these are results for last circular
t: Cirt 460 LRTE PPP link
https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb.333a_.gif
I
wish to know if this result is good for an ensemble like we  have here for
starting this discussion...

Given you have only a single Cs beam standard, this looks ok and
in the order of magnitude I would expect the stability of the Cs beam.

The BVA only contributes to short term stability and thus does not
make a difference in the Circular T plots.

And what you all suggest for improvement.

This depends a lot on what you want to achieve.
Is it short term performance you are after? Is it long term stability?
Is it reliability? Is it lower uncertainty to UTC?

Quite honestly, given that you are an NMI and we are talking about
a national timescale, I would recommend that you first try to enhance
your resilience against device failures. Having only a single Cs beam
standard, which need a replacement tube every 5 to 20 years (depending
on type and chance), you run the risk of losing your timescale when your
Cs beam standard runs out of Cs.

Today i have:

Real time tropospheric delay calculation with hopfield's model to replace
"MDTR" (with also mapping function to correct for each satellite). Every 15
minutes, also, I fed the Rx5Tr receiver with temperature, humidity and
pressure for its tropospheric model update. The sensor is located near the
antenna.

At the current state, I am not sure whether GNSS time transfer is
really the limiting factor for you. At least not short term.
IIRC the current uncertainty for GNSS time transfer is around 2ns,
even with iPPP, because of delay stability in the device itself.
Of course, if you can make your antenna's filter more stable, you
would then be able to get better absolute calibration.

And an algorithm that simply sees the frequency deviation every 2 hours and
computes a frequency correction for our HROG-5.

Given your MDEV data, I would set the correction time-span to 1-2days.
At least, that's where your MDEV flattens out.

We also have a hydrogen maser that is stopped because the 10 MHz oscillator
is not locking. I want to do some maintenance there to see if it can be
brought back to life.

The maser is glowing purple, but it shows "no vacuum" and "synthesizer is
faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the
cavity output, but nothing more.

So, if possible, I may want to be guided in some steps to see if is it
possible to recover it.

We have had some time-nuts members repair their H-Masers on their own.
But given that you are an NMI, I would contact the manufacturer. They
are most likely willing to help.

I hope this helps

			Attila Kinali

--
The driving force behind research is the question: "Why?"
There are things we don't understand and things we always
wonder about. And that's why we do research.
-- Kobayashi Makoto

A wonderful good morning! On Mon, 25 May 2026 15:38:54 -0300 Luiz Paulo Damaceno via time-nuts <time-nuts@lists.febo.com> wrote: > I've started to see if is possible to fix an H-maser that we have here in > our timelab. Today we're contributing to UTC With some ensemble that is > composed by: 1 commercial cs clock + BVA phase locked in long term (<100s) > to the cs + synthesizer + HROG-5. And these are results for last circular > t: Cirt 460 LRTE PPP link > <https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb.333a_.gif> > I > wish to know if this result is good for an ensemble like we have here for > starting this discussion... Given you have only a single Cs beam standard, this looks ok and in the order of magnitude I would expect the stability of the Cs beam. The BVA only contributes to short term stability and thus does not make a difference in the Circular T plots. > And what you all suggest for improvement. This depends a lot on what you want to achieve. Is it short term performance you are after? Is it long term stability? Is it reliability? Is it lower uncertainty to UTC? Quite honestly, given that you are an NMI and we are talking about a national timescale, I would recommend that you first try to enhance your resilience against device failures. Having only a single Cs beam standard, which need a replacement tube every 5 to 20 years (depending on type and chance), you run the risk of losing your timescale when your Cs beam standard runs out of Cs. > Today i have: > > Real time tropospheric delay calculation with hopfield's model to replace > "MDTR" (with also mapping function to correct for each satellite). Every 15 > minutes, also, I fed the Rx5Tr receiver with temperature, humidity and > pressure for its tropospheric model update. The sensor is located near the > antenna. At the current state, I am not sure whether GNSS time transfer is really the limiting factor for you. At least not short term. IIRC the current uncertainty for GNSS time transfer is around 2ns, even with iPPP, because of delay stability in the device itself. Of course, if you can make your antenna's filter more stable, you would then be able to get better absolute calibration. > And an algorithm that simply sees the frequency deviation every 2 hours and > computes a frequency correction for our HROG-5. Given your MDEV data, I would set the correction time-span to 1-2days. At least, that's where your MDEV flattens out. > We also have a hydrogen maser that is stopped because the 10 MHz oscillator > is not locking. I want to do some maintenance there to see if it can be > brought back to life. > > The maser is glowing purple, but it shows "no vacuum" and "synthesizer is > faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the > cavity output, but nothing more. > > So, if possible, I may want to be guided in some steps to see if is it > possible to recover it. We have had some time-nuts members repair their H-Masers on their own. But given that you are an NMI, I would contact the manufacturer. They are most likely willing to help. I hope this helps Attila Kinali -- The driving force behind research is the question: "Why?" There are things we don't understand and things we always wonder about. And that's why we do research. -- Kobayashi Makoto
LP
Luiz Paulo Damaceno
Tue, May 26, 2026 1:15 PM

John,

-> The Cs+GNSS ensemble looks like it's performing very well.  That's the
Septentrio PolaRx5TR receiver, correct?
That's correct.

-> It sounds like you may have a power supply problem with the maser, or
perhaps a controller issue, since you obviously have vacuum if the
dissociator is lit.  How far off frequency is it?  More than a few Hz
suggests that the oscillator oven has failed, which could explain everything
except the vacuum error.

Is not that too far, I can manually adjust the frequency and stability
seems quite good (unlocked PolaRx5Tr shows something around 4~3E-12 for 1s
ADEV).
Did you think checking power supply voltages (not trusting the display in
the instrument front).

Thanks

Luiz Paulo

Em ter., 26 de mai. de 2026 às 02:48, john@miles.io escreveu:

The Cs+GNSS ensemble looks like it's performing very well.  That's the
Septentrio PolaRx5TR receiver, correct?

It sounds like you may have a power supply problem with the maser, or
perhaps a controller issue, since you obviously have vacuum if the
dissociator is lit.  How far off frequency is it?  More than a few Hz
suggests that the oscillator oven has failed, which could explain
everything
except the vacuum error.

-- john

-----Original Message-----
From: Luiz Paulo Damaceno via time-nuts time-nuts@lists.febo.com
Sent: Monday, May 25, 2026 11:39 AM
To: Discussion of precise time and frequency measurement
time-nuts@lists.febo.com
Cc: Luiz Paulo Damaceno luizpauloeletrico42@gmail.com
Subject: [time-nuts] UTC(LRTE) H-Maser maintenace

Hi all,

I've started to see if is possible to fix an H-maser that we have here in
our timelab. Today we're contributing to UTC With some ensemble that is
composed by: 1 commercial cs clock + BVA phase locked in long term (<100s)
to the cs + synthesizer + HROG-5. And these are results for last circular
t: Cirt 460 LRTE PPP link
<
https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb.
333a_.gif
https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb.333a_.gif

I
wish to know if this result is good for an ensemble like we  have here for
starting this discussion... And what you all suggest for improvement. Today
i have:

Real time tropospheric delay calculation with hopfield's model to replace
"MDTR" (with also mapping function to correct for each satellite). Every 15
minutes, also, I fed the Rx5Tr receiver with temperature, humidity and
pressure for its tropospheric model update. The sensor is located near the
antenna.

And an algorithm that simply sees the frequency deviation every 2 hours and
computes a frequency correction for our HROG-5.

We also have a hydrogen maser that is stopped because the 10 MHz oscillator
is not locking. I want to do some maintenance there to see if it can be
brought back to life.

The maser is glowing purple, but it shows "no vacuum" and "synthesizer is
faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the
cavity output, but nothing more.

So, if possible, I may want to be guided in some steps to see if is it
possible to recover it.

Best regards,

Luiz


time-nuts mailing list -- time-nuts@lists.febo.com To unsubscribe send an
email to time-nuts-leave@lists.febo.com

John, -> The Cs+GNSS ensemble looks like it's performing very well. That's the Septentrio PolaRx5TR receiver, correct? That's correct. -> It sounds like you may have a power supply problem with the maser, or perhaps a controller issue, since you obviously have vacuum if the dissociator is lit. How far off frequency is it? More than a few Hz suggests that the oscillator oven has failed, which could explain everything except the vacuum error. Is not that too far, I can manually adjust the frequency and stability seems quite good (unlocked PolaRx5Tr shows something around 4~3E-12 for 1s ADEV). Did you think checking power supply voltages (not trusting the display in the instrument front). Thanks Luiz Paulo Em ter., 26 de mai. de 2026 às 02:48, <john@miles.io> escreveu: > The Cs+GNSS ensemble looks like it's performing very well. That's the > Septentrio PolaRx5TR receiver, correct? > > It sounds like you may have a power supply problem with the maser, or > perhaps a controller issue, since you obviously have vacuum if the > dissociator is lit. How far off frequency is it? More than a few Hz > suggests that the oscillator oven has failed, which could explain > everything > except the vacuum error. > > -- john > > -----Original Message----- > From: Luiz Paulo Damaceno via time-nuts <time-nuts@lists.febo.com> > Sent: Monday, May 25, 2026 11:39 AM > To: Discussion of precise time and frequency measurement > <time-nuts@lists.febo.com> > Cc: Luiz Paulo Damaceno <luizpauloeletrico42@gmail.com> > Subject: [time-nuts] UTC(LRTE) H-Maser maintenace > > Hi all, > > I've started to see if is possible to fix an H-maser that we have here in > our timelab. Today we're contributing to UTC With some ensemble that is > composed by: 1 commercial cs clock + BVA phase locked in long term (<100s) > to the cs + synthesizer + HROG-5. And these are results for last circular > t: Cirt 460 LRTE PPP link > < > https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb. > 333a_.gif > <https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb.333a_.gif> > > > I > wish to know if this result is good for an ensemble like we have here for > starting this discussion... And what you all suggest for improvement. Today > i have: > > Real time tropospheric delay calculation with hopfield's model to replace > "MDTR" (with also mapping function to correct for each satellite). Every 15 > minutes, also, I fed the Rx5Tr receiver with temperature, humidity and > pressure for its tropospheric model update. The sensor is located near the > antenna. > > And an algorithm that simply sees the frequency deviation every 2 hours and > computes a frequency correction for our HROG-5. > > We also have a hydrogen maser that is stopped because the 10 MHz oscillator > is not locking. I want to do some maintenance there to see if it can be > brought back to life. > > The maser is glowing purple, but it shows "no vacuum" and "synthesizer is > faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the > cavity output, but nothing more. > > So, if possible, I may want to be guided in some steps to see if is it > possible to recover it. > > Best regards, > > Luiz > _______________________________________________ > time-nuts mailing list -- time-nuts@lists.febo.com To unsubscribe send an > email to time-nuts-leave@lists.febo.com > >
LP
Luiz Paulo Damaceno
Tue, May 26, 2026 1:21 PM

Thank you, Attila!

-> I want to achieve long term stability and also short term performance. I
think both are important to us. I can figure out that things better than we
have now may need more clocks or a change of base clock.

-> Quite honestly, given that you are an NMI and we are talking about
a national timescale, I would recommend that you first try to enhance
your resilience against device failures. Having only a single Cs beam
standard, which need a replacement tube every 5 to 20 years (depending
on type and chance), you run the risk of losing your timescale when your
Cs beam standard runs out of Cs.

  • I'm not an NMI, I'm in a university that runs atomic physics
    experiments. Our UTC time scale is one way for us to have trackability to
    Cs frequency realization.
  • Actually we have a second Cs beam that is not running due to this: have
    a second one in case of failure, at least.

Thank you for your answers,

Luiz Paulo

Em ter., 26 de mai. de 2026 às 06:56, Attila Kinali via time-nuts <
time-nuts@lists.febo.com> escreveu:

A wonderful good morning!

On Mon, 25 May 2026 15:38:54 -0300
Luiz Paulo Damaceno via time-nuts time-nuts@lists.febo.com wrote:

I've started to see if is possible to fix an H-maser that we have here in
our timelab. Today we're contributing to UTC With some ensemble that is
composed by: 1 commercial cs clock + BVA phase locked in long term

(<100s)

to the cs + synthesizer + HROG-5. And these are results for last circular
t: Cirt 460 LRTE PPP link
<

I
wish to know if this result is good for an ensemble like we  have here

for

starting this discussion...

Given you have only a single Cs beam standard, this looks ok and
in the order of magnitude I would expect the stability of the Cs beam.

The BVA only contributes to short term stability and thus does not
make a difference in the Circular T plots.

And what you all suggest for improvement.

This depends a lot on what you want to achieve.
Is it short term performance you are after? Is it long term stability?
Is it reliability? Is it lower uncertainty to UTC?

Quite honestly, given that you are an NMI and we are talking about
a national timescale, I would recommend that you first try to enhance
your resilience against device failures. Having only a single Cs beam
standard, which need a replacement tube every 5 to 20 years (depending
on type and chance), you run the risk of losing your timescale when your
Cs beam standard runs out of Cs.

Today i have:

Real time tropospheric delay calculation with hopfield's model to replace
"MDTR" (with also mapping function to correct for each satellite). Every

15

minutes, also, I fed the Rx5Tr receiver with temperature, humidity and
pressure for its tropospheric model update. The sensor is located near

the

antenna.

At the current state, I am not sure whether GNSS time transfer is
really the limiting factor for you. At least not short term.
IIRC the current uncertainty for GNSS time transfer is around 2ns,
even with iPPP, because of delay stability in the device itself.
Of course, if you can make your antenna's filter more stable, you
would then be able to get better absolute calibration.

And an algorithm that simply sees the frequency deviation every 2 hours

and

computes a frequency correction for our HROG-5.

Given your MDEV data, I would set the correction time-span to 1-2days.
At least, that's where your MDEV flattens out.

We also have a hydrogen maser that is stopped because the 10 MHz

oscillator

is not locking. I want to do some maintenance there to see if it can be
brought back to life.

The maser is glowing purple, but it shows "no vacuum" and "synthesizer is
faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the
cavity output, but nothing more.

So, if possible, I may want to be guided in some steps to see if is it
possible to recover it.

We have had some time-nuts members repair their H-Masers on their own.
But given that you are an NMI, I would contact the manufacturer. They
are most likely willing to help.

I hope this helps

                             Attila Kinali

--
The driving force behind research is the question: "Why?"
There are things we don't understand and things we always
wonder about. And that's why we do research.
-- Kobayashi Makoto


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Thank you, Attila! -> I want to achieve long term stability and also short term performance. I think both are important to us. I can figure out that things better than we have now may need more clocks or a change of base clock. -> Quite honestly, given that you are an NMI and we are talking about a national timescale, I would recommend that you first try to enhance your resilience against device failures. Having only a single Cs beam standard, which need a replacement tube every 5 to 20 years (depending on type and chance), you run the risk of losing your timescale when your Cs beam standard runs out of Cs. - I'm not an NMI, I'm in a university that runs atomic physics experiments. Our UTC time scale is one way for us to have trackability to Cs frequency realization. - Actually we have a second Cs beam that is not running due to this: have a second one in case of failure, at least. Thank you for your answers, Luiz Paulo Em ter., 26 de mai. de 2026 às 06:56, Attila Kinali via time-nuts < time-nuts@lists.febo.com> escreveu: > A wonderful good morning! > > On Mon, 25 May 2026 15:38:54 -0300 > Luiz Paulo Damaceno via time-nuts <time-nuts@lists.febo.com> wrote: > > > I've started to see if is possible to fix an H-maser that we have here in > > our timelab. Today we're contributing to UTC With some ensemble that is > > composed by: 1 commercial cs clock + BVA phase locked in long term > (<100s) > > to the cs + synthesizer + HROG-5. And these are results for last circular > > t: Cirt 460 LRTE PPP link > > < > https://webtai.bipm.org/ftp/pub/tai/timelinks/lkc/2604/lrteptb/lnk/lrteptb.333a_.gif > > > > I > > wish to know if this result is good for an ensemble like we have here > for > > starting this discussion... > > Given you have only a single Cs beam standard, this looks ok and > in the order of magnitude I would expect the stability of the Cs beam. > > The BVA only contributes to short term stability and thus does not > make a difference in the Circular T plots. > > > And what you all suggest for improvement. > > This depends a lot on what you want to achieve. > Is it short term performance you are after? Is it long term stability? > Is it reliability? Is it lower uncertainty to UTC? > > Quite honestly, given that you are an NMI and we are talking about > a national timescale, I would recommend that you first try to enhance > your resilience against device failures. Having only a single Cs beam > standard, which need a replacement tube every 5 to 20 years (depending > on type and chance), you run the risk of losing your timescale when your > Cs beam standard runs out of Cs. > > > Today i have: > > > > Real time tropospheric delay calculation with hopfield's model to replace > > "MDTR" (with also mapping function to correct for each satellite). Every > 15 > > minutes, also, I fed the Rx5Tr receiver with temperature, humidity and > > pressure for its tropospheric model update. The sensor is located near > the > > antenna. > > At the current state, I am not sure whether GNSS time transfer is > really the limiting factor for you. At least not short term. > IIRC the current uncertainty for GNSS time transfer is around 2ns, > even with iPPP, because of delay stability in the device itself. > Of course, if you can make your antenna's filter more stable, you > would then be able to get better absolute calibration. > > > > And an algorithm that simply sees the frequency deviation every 2 hours > and > > computes a frequency correction for our HROG-5. > > Given your MDEV data, I would set the correction time-span to 1-2days. > At least, that's where your MDEV flattens out. > > > We also have a hydrogen maser that is stopped because the 10 MHz > oscillator > > is not locking. I want to do some maintenance there to see if it can be > > brought back to life. > > > > The maser is glowing purple, but it shows "no vacuum" and "synthesizer is > > faulty". I can see an A.M. oscillation of about -140 to -120 dBm in the > > cavity output, but nothing more. > > > > So, if possible, I may want to be guided in some steps to see if is it > > possible to recover it. > > We have had some time-nuts members repair their H-Masers on their own. > But given that you are an NMI, I would contact the manufacturer. They > are most likely willing to help. > > I hope this helps > > Attila Kinali > > -- > The driving force behind research is the question: "Why?" > There are things we don't understand and things we always > wonder about. And that's why we do research. > -- Kobayashi Makoto > _______________________________________________ > time-nuts mailing list -- time-nuts@lists.febo.com > To unsubscribe send an email to time-nuts-leave@lists.febo.com >
AK
Attila Kinali
Tue, May 26, 2026 2:27 PM

Ola Luiz Paulo!

On Tue, 26 May 2026 10:21:03 -0300
Luiz Paulo Damaceno luizpauloeletrico42@gmail.com wrote:

-> I want to achieve long term stability and also short term performance.
I think both are important to us. I can figure out that things better than we
have now may need more clocks or a change of base clock.

Ok. One "easy" first thing you can do is to more loosely couple
your BVA to your Cs beam standard. If your BVA is well aged,
it is likely to perform better than the Cs beam standard up
to 1000s. If you change the loop-bandwidth of your PLL such
that you get somewhere between 0.01Hz and 0.001Hz, then you
could make better use of your BVA. Of course, that's not
as easy as it sounds. If you have some phase measurement
equipment (e.g. a Timepod, but also a red pitaya would probably
do), you could use the BVA as input to the HROG, then compare
the phase of the HROG output and the Cs beam standard. It would
be then pretty easy to do the PLL loop on some PC and use the
HROG for the control/feedback part.

-> Quite honestly, given that you are an NMI and we are talking about
a national timescale, I would recommend that you first try to enhance
your resilience against device failures. Having only a single Cs beam
standard, which need a replacement tube every 5 to 20 years (depending
on type and chance), you run the risk of losing your timescale when your
Cs beam standard runs out of Cs.

  • I'm not an NMI, I'm in a university that runs atomic physics
    experiments.

Oh.. sorry. My apologies! I assumed that you were an NMI as it is
rare that non-NMIs contribute to TAI/UTC.

Our UTC time scale is one way for us to have trackability to
Cs frequency realization.

  • Actually we have a second Cs beam that is not running due to this: have
    a second one in case of failure, at least.

Ok, so you don't have any legal requirement to keep a continuous
timescale. I guess your primary need is to provide a local realization
of the SI second that is as accurate as possible with as little noise
and uncertainty as possible?

Then I would focus on getting the hydrogen maser working again
and use it as input to the HROG. That will provide you the best
short to medium term performance.

Then use your phase meter to compare your HROG output and the
Cs beam output. This way you can correct for the drift of the
maser. Use the GNSS system to correct the drift of the Cs beam
standard with a tau in the range of a few weeks to a month.

This is basically what METAS does (minus the Cs fountain that
they periodically run) [1].

BTW: If your research involves optical atomic clocks and their
absolute frequency measurement, you might want to consider getting
a primary frequency standard. In the course of the presentation on the
2025 BIPM recommended frequency list at EFTF last month, Helen Margolis
from NPL did complain about the correlations of absolute frequency
measurements done through UTC, which are very hard to properly handle.

		Attila Kinali

[1] "METAS new time scale generation system - A progress report"
by Bernier, Dudle and Schlunegger, 2006
http://time.kinali.ch/ptti/2006papers/paper3.pdf

The driving force behind research is the question: "Why?"
There are things we don't understand and things we always
wonder about. And that's why we do research.
-- Kobayashi Makoto

Ola Luiz Paulo! On Tue, 26 May 2026 10:21:03 -0300 Luiz Paulo Damaceno <luizpauloeletrico42@gmail.com> wrote: > -> I want to achieve long term stability and also short term performance. > I think both are important to us. I can figure out that things better than we > have now may need more clocks or a change of base clock. Ok. One "easy" first thing you can do is to more loosely couple your BVA to your Cs beam standard. If your BVA is well aged, it is likely to perform better than the Cs beam standard up to 1000s. If you change the loop-bandwidth of your PLL such that you get somewhere between 0.01Hz and 0.001Hz, then you could make better use of your BVA. Of course, that's not as easy as it sounds. If you have some phase measurement equipment (e.g. a Timepod, but also a red pitaya would probably do), you could use the BVA as input to the HROG, then compare the phase of the HROG output and the Cs beam standard. It would be then pretty easy to do the PLL loop on some PC and use the HROG for the control/feedback part. > -> Quite honestly, given that you are an NMI and we are talking about > a national timescale, I would recommend that you first try to enhance > your resilience against device failures. Having only a single Cs beam > standard, which need a replacement tube every 5 to 20 years (depending > on type and chance), you run the risk of losing your timescale when your > Cs beam standard runs out of Cs. > - I'm not an NMI, I'm in a university that runs atomic physics > experiments. Oh.. sorry. My apologies! I assumed that you were an NMI as it is rare that non-NMIs contribute to TAI/UTC. > Our UTC time scale is one way for us to have trackability to > Cs frequency realization. > - Actually we have a second Cs beam that is not running due to this: have > a second one in case of failure, at least. Ok, so you don't have any legal requirement to keep a continuous timescale. I guess your primary need is to provide a local realization of the SI second that is as accurate as possible with as little noise and uncertainty as possible? Then I would focus on getting the hydrogen maser working again and use it as input to the HROG. That will provide you the best short to medium term performance. Then use your phase meter to compare your HROG output and the Cs beam output. This way you can correct for the drift of the maser. Use the GNSS system to correct the drift of the Cs beam standard with a tau in the range of a few weeks to a month. This is basically what METAS does (minus the Cs fountain that they periodically run) [1]. BTW: If your research involves optical atomic clocks and their absolute frequency measurement, you might want to consider getting a primary frequency standard. In the course of the presentation on the 2025 BIPM recommended frequency list at EFTF last month, Helen Margolis from NPL did complain about the correlations of absolute frequency measurements done through UTC, which are very hard to properly handle. Attila Kinali [1] "METAS new time scale generation system - A progress report" by Bernier, Dudle and Schlunegger, 2006 http://time.kinali.ch/ptti/2006papers/paper3.pdf -- The driving force behind research is the question: "Why?" There are things we don't understand and things we always wonder about. And that's why we do research. -- Kobayashi Makoto
J
john@miles.io
Tue, May 26, 2026 4:16 PM

Hard to say without knowing anything about the unit in question, but it’s not a bad idea to look at the supply rails with an actual DMM or scope.  Depending on resolution, sampling rate and smoothing, ripple or noise/instability may not get flagged by the self-monitoring hardware.

I think I’d focus on the vacuum failure message after that.  Is it just complaining that the ion pump current is slightly high, or is it actually reading a separate vacuum gauge and not liking what it sees?  A false report might be a clue to the same problem that keeps the control loop from locking.  At the same time, maybe the vacuum integrity is good enough to allow the H2 dissociator to light up, but not good enough to support maser action.

If it’s an active maser and you are seeing any signal at all from the cavity, that sounds like a good sign.  If it’s a passive maser, there will always be some 1420 MHz output as long as the input port is driven, so that wouldn’t necessarily tell you much.

-- john

From: Luiz Paulo Damaceno luizpauloeletrico42@gmail.com

Is not that too far, I can manually adjust the frequency and stability seems quite good (unlocked PolaRx5Tr shows something around 4~3E-12 for 1s ADEV).

Did you think checking power supply voltages (not trusting the display in the instrument front).

Hard to say without knowing anything about the unit in question, but it’s not a bad idea to look at the supply rails with an actual DMM or scope. Depending on resolution, sampling rate and smoothing, ripple or noise/instability may not get flagged by the self-monitoring hardware. I think I’d focus on the vacuum failure message after that. Is it just complaining that the ion pump current is slightly high, or is it actually reading a separate vacuum gauge and not liking what it sees? A false report might be a clue to the same problem that keeps the control loop from locking. At the same time, maybe the vacuum integrity is good enough to allow the H2 dissociator to light up, but not good enough to support maser action. If it’s an active maser and you are seeing any signal at all from the cavity, that sounds like a good sign. If it’s a passive maser, there will always be some 1420 MHz output as long as the input port is driven, so that wouldn’t necessarily tell you much. -- john From: Luiz Paulo Damaceno <luizpauloeletrico42@gmail.com> Is not that too far, I can manually adjust the frequency and stability seems quite good (unlocked PolaRx5Tr shows something around 4~3E-12 for 1s ADEV). Did you think checking power supply voltages (not trusting the display in the instrument front).
LP
Luiz Paulo Damaceno
Thu, May 28, 2026 1:37 PM

Ola, Attila!

Ok. One "easy" first thing you can do is to more loosely couple
your BVA to your Cs beam standard. If your BVA is well aged,
it is likely to perform better than the Cs beam standard up
to 1000s. If you change the loop-bandwidth of your PLL such
that you get somewhere between 0.01Hz and 0.001Hz, then you
could make better use of your BVA. Of course, that's not
as easy as it sounds. If you have some phase measurement
equipment (e.g. a Timepod, but also a red pitaya would probably
do), you could use the BVA as input to the HROG, then compare
the phase of the HROG output and the Cs beam standard. It would
be then pretty easy to do the PLL loop on some PC and use the
HROG for the control/feedback part.

Thank you for the considerations. I've tunned the PLL for 0.00289Hz, today
i'm using a 1,1M ohm resistance and 50 uF capacitor. I can also reduce the
error voltage by changing the voltage in a potentiometer, just like a
"volume" control in audio systems. I expect to reduce a bit 0,25 times day
to day) to archive 1000s loop. I can only evaluate this using GNSS PPP - by
RTKLib in real time or NRCAN for example and / or CGGTTS files.

I have also available for these measurements a frequency comb from menlo
systems. Can I use repetition rate adev to evaluate the BVA? (locking it in
a Cs beam and then in BVA + Cs beam)?

Ok, so you don't have any legal requirement to keep a continuous
timescale. I guess your primary need is to provide a local realization
of the SI second that is as accurate as possible with as little noise
and uncertainty as possible?

Yes, no legal requirement, here in Brazil, only ONJR has the legal
requirement. Yes, my primary need is to provide a local realization of SI
second with little noise and uncertainty.

We are working in cold atom clocks here also. A Cs fountain and another
kind of cold atom Cs clock. But now, we're in the construction phase. No
measurements being made.

About getting the maser working again, do you have any experience with that
maser? Is the KVARZ CH1-75A.

Abraços,

Luiz Paulo

Em ter., 26 de mai. de 2026 às 11:27, Attila Kinali attila@kinali.ch
escreveu:

Ola Luiz Paulo!

On Tue, 26 May 2026 10:21:03 -0300
Luiz Paulo Damaceno luizpauloeletrico42@gmail.com wrote:

-> I want to achieve long term stability and also short term

performance.

I think both are important to us. I can figure out that things better

than we

have now may need more clocks or a change of base clock.

Ok. One "easy" first thing you can do is to more loosely couple
your BVA to your Cs beam standard. If your BVA is well aged,
it is likely to perform better than the Cs beam standard up
to 1000s. If you change the loop-bandwidth of your PLL such
that you get somewhere between 0.01Hz and 0.001Hz, then you
could make better use of your BVA. Of course, that's not
as easy as it sounds. If you have some phase measurement
equipment (e.g. a Timepod, but also a red pitaya would probably
do), you could use the BVA as input to the HROG, then compare
the phase of the HROG output and the Cs beam standard. It would
be then pretty easy to do the PLL loop on some PC and use the
HROG for the control/feedback part.

-> Quite honestly, given that you are an NMI and we are talking about
a national timescale, I would recommend that you first try to enhance
your resilience against device failures. Having only a single Cs beam
standard, which need a replacement tube every 5 to 20 years (depending
on type and chance), you run the risk of losing your timescale when your
Cs beam standard runs out of Cs.

  • I'm not an NMI, I'm in a university that runs atomic physics
    experiments.

Oh.. sorry. My apologies! I assumed that you were an NMI as it is
rare that non-NMIs contribute to TAI/UTC.

Our UTC time scale is one way for us to have trackability to
Cs frequency realization.

  • Actually we have a second Cs beam that is not running due to this:

have

a second one in case of failure, at least.

Ok, so you don't have any legal requirement to keep a continuous
timescale. I guess your primary need is to provide a local realization
of the SI second that is as accurate as possible with as little noise
and uncertainty as possible?

Then I would focus on getting the hydrogen maser working again
and use it as input to the HROG. That will provide you the best
short to medium term performance.

Then use your phase meter to compare your HROG output and the
Cs beam output. This way you can correct for the drift of the
maser. Use the GNSS system to correct the drift of the Cs beam
standard with a tau in the range of a few weeks to a month.

This is basically what METAS does (minus the Cs fountain that
they periodically run) [1].

BTW: If your research involves optical atomic clocks and their
absolute frequency measurement, you might want to consider getting
a primary frequency standard. In the course of the presentation on the
2025 BIPM recommended frequency list at EFTF last month, Helen Margolis
from NPL did complain about the correlations of absolute frequency
measurements done through UTC, which are very hard to properly handle.

                     Attila Kinali

[1] "METAS new time scale generation system - A progress report"
by Bernier, Dudle and Schlunegger, 2006
http://time.kinali.ch/ptti/2006papers/paper3.pdf

The driving force behind research is the question: "Why?"
There are things we don't understand and things we always
wonder about. And that's why we do research.
-- Kobayashi Makoto

Ola, Attila! >Ok. One "easy" first thing you can do is to more loosely couple >your BVA to your Cs beam standard. If your BVA is well aged, >it is likely to perform better than the Cs beam standard up >to 1000s. If you change the loop-bandwidth of your PLL such >that you get somewhere between 0.01Hz and 0.001Hz, then you >could make better use of your BVA. Of course, that's not >as easy as it sounds. If you have some phase measurement >equipment (e.g. a Timepod, but also a red pitaya would probably >do), you could use the BVA as input to the HROG, then compare >the phase of the HROG output and the Cs beam standard. It would >be then pretty easy to do the PLL loop on some PC and use the >HROG for the control/feedback part. Thank you for the considerations. I've tunned the PLL for 0.00289Hz, today i'm using a 1,1M ohm resistance and 50 uF capacitor. I can also reduce the error voltage by changing the voltage in a potentiometer, just like a "volume" control in audio systems. I expect to reduce a bit 0,25 times day to day) to archive 1000s loop. I can only evaluate this using GNSS PPP - by RTKLib in real time or NRCAN for example and / or CGGTTS files. I have also available for these measurements a frequency comb from menlo systems. Can I use repetition rate adev to evaluate the BVA? (locking it in a Cs beam and then in BVA + Cs beam)? >Ok, so you don't have any legal requirement to keep a continuous >timescale. I guess your primary need is to provide a local realization >of the SI second that is as accurate as possible with as little noise >and uncertainty as possible? Yes, no legal requirement, here in Brazil, only ONJR has the legal requirement. Yes, my primary need is to provide a local realization of SI second with little noise and uncertainty. We are working in cold atom clocks here also. A Cs fountain and another kind of cold atom Cs clock. But now, we're in the construction phase. No measurements being made. About getting the maser working again, do you have any experience with that maser? Is the KVARZ CH1-75A. Abraços, Luiz Paulo Em ter., 26 de mai. de 2026 às 11:27, Attila Kinali <attila@kinali.ch> escreveu: > Ola Luiz Paulo! > > On Tue, 26 May 2026 10:21:03 -0300 > Luiz Paulo Damaceno <luizpauloeletrico42@gmail.com> wrote: > > > -> I want to achieve long term stability and also short term > performance. > > I think both are important to us. I can figure out that things better > than we > > have now may need more clocks or a change of base clock. > > Ok. One "easy" first thing you can do is to more loosely couple > your BVA to your Cs beam standard. If your BVA is well aged, > it is likely to perform better than the Cs beam standard up > to 1000s. If you change the loop-bandwidth of your PLL such > that you get somewhere between 0.01Hz and 0.001Hz, then you > could make better use of your BVA. Of course, that's not > as easy as it sounds. If you have some phase measurement > equipment (e.g. a Timepod, but also a red pitaya would probably > do), you could use the BVA as input to the HROG, then compare > the phase of the HROG output and the Cs beam standard. It would > be then pretty easy to do the PLL loop on some PC and use the > HROG for the control/feedback part. > > > -> Quite honestly, given that you are an NMI and we are talking about > > a national timescale, I would recommend that you first try to enhance > > your resilience against device failures. Having only a single Cs beam > > standard, which need a replacement tube every 5 to 20 years (depending > > on type and chance), you run the risk of losing your timescale when your > > Cs beam standard runs out of Cs. > > - I'm not an NMI, I'm in a university that runs atomic physics > > experiments. > > Oh.. sorry. My apologies! I assumed that you were an NMI as it is > rare that non-NMIs contribute to TAI/UTC. > > > Our UTC time scale is one way for us to have trackability to > > Cs frequency realization. > > - Actually we have a second Cs beam that is not running due to this: > have > > a second one in case of failure, at least. > > Ok, so you don't have any legal requirement to keep a continuous > timescale. I guess your primary need is to provide a local realization > of the SI second that is as accurate as possible with as little noise > and uncertainty as possible? > > Then I would focus on getting the hydrogen maser working again > and use it as input to the HROG. That will provide you the best > short to medium term performance. > > Then use your phase meter to compare your HROG output and the > Cs beam output. This way you can correct for the drift of the > maser. Use the GNSS system to correct the drift of the Cs beam > standard with a tau in the range of a few weeks to a month. > > This is basically what METAS does (minus the Cs fountain that > they periodically run) [1]. > > BTW: If your research involves optical atomic clocks and their > absolute frequency measurement, you might want to consider getting > a primary frequency standard. In the course of the presentation on the > 2025 BIPM recommended frequency list at EFTF last month, Helen Margolis > from NPL did complain about the correlations of absolute frequency > measurements done through UTC, which are very hard to properly handle. > > > Attila Kinali > > > [1] "METAS new time scale generation system - A progress report" > by Bernier, Dudle and Schlunegger, 2006 > http://time.kinali.ch/ptti/2006papers/paper3.pdf > -- > The driving force behind research is the question: "Why?" > There are things we don't understand and things we always > wonder about. And that's why we do research. > -- Kobayashi Makoto >
LP
Luiz Paulo Damaceno
Thu, May 28, 2026 1:39 PM

Thank you john!

I will verify supply rails with DMM / scope and return the results. For
now, Is it an active maser unit. CH1-75A from KVARZ.

Kind regards,

Luiz Paulo

Em ter., 26 de mai. de 2026 às 13:16, john@miles.io escreveu:

Hard to say without knowing anything about the unit in question, but it’s
not a bad idea to look at the supply rails with an actual DMM or scope.
Depending on resolution, sampling rate and smoothing, ripple or
noise/instability may not get flagged by the self-monitoring hardware.

I think I’d focus on the vacuum failure message after that.  Is it just
complaining that the ion pump current is slightly high, or is it actually
reading a separate vacuum gauge and not liking what it sees?  A false
report might be a clue to the same problem that keeps the control loop from
locking.  At the same time, maybe the vacuum integrity is good enough to
allow the H2 dissociator to light up, but not good enough to support maser
action.

If it’s an active maser and you are seeing any signal at all from the
cavity, that sounds like a good sign.  If it’s a passive maser, there will
always be some 1420 MHz output as long as the input port is driven, so that
wouldn’t necessarily tell you much.

-- john

From: Luiz Paulo Damaceno luizpauloeletrico42@gmail.com

Is not that too far, I can manually adjust the frequency and stability
seems quite good (unlocked PolaRx5Tr shows something around 4~3E-12 for 1s
ADEV).

Did you think checking power supply voltages (not trusting the display in
the instrument front).

Thank you john! I will verify supply rails with DMM / scope and return the results. For now, Is it an active maser unit. CH1-75A from KVARZ. Kind regards, Luiz Paulo Em ter., 26 de mai. de 2026 às 13:16, <john@miles.io> escreveu: > Hard to say without knowing anything about the unit in question, but it’s > not a bad idea to look at the supply rails with an actual DMM or scope. > Depending on resolution, sampling rate and smoothing, ripple or > noise/instability may not get flagged by the self-monitoring hardware. > > > > I think I’d focus on the vacuum failure message after that. Is it just > complaining that the ion pump current is slightly high, or is it actually > reading a separate vacuum gauge and not liking what it sees? A false > report might be a clue to the same problem that keeps the control loop from > locking. At the same time, maybe the vacuum integrity is good enough to > allow the H2 dissociator to light up, but not good enough to support maser > action. > > > > If it’s an active maser and you are seeing any signal at all from the > cavity, that sounds like a good sign. If it’s a passive maser, there will > always be some 1420 MHz output as long as the input port is driven, so that > wouldn’t necessarily tell you much. > > > > -- john > > > > > > *From:* Luiz Paulo Damaceno <luizpauloeletrico42@gmail.com> > > Is not that too far, I can manually adjust the frequency and stability > seems quite good (unlocked PolaRx5Tr shows something around 4~3E-12 for 1s > ADEV). > > Did you think checking power supply voltages (not trusting the display in > the instrument front). >
AK
Attila Kinali
Thu, May 28, 2026 3:30 PM

A wonderful good afternoon,

On Thu, 28 May 2026 10:37:58 -0300
Luiz Paulo Damaceno via time-nuts time-nuts@lists.febo.com wrote:

Thank you for the considerations. I've tunned the PLL for 0.00289Hz, today
i'm using a 1,1M ohm resistance and 50 uF capacitor. I can also reduce the
error voltage by changing the voltage in a potentiometer, just like a
"volume" control in audio systems. I expect to reduce a bit 0,25 times day
to day) to archive 1000s loop.

A PLL using the EFC input of the BVA will not work well at these
long time constants. About 1Hz loop bandwidth is the lowest that's
reasonable, I would even draw the line at 10Hz. And only if you
build an active filter using an low-noise opamp. Going lower will
limit your oscillators stability by the noise on the EFC voltage.
You have a 1MΩ resistor, which already produces quite a bit of
noise voltage. And then you use a 50µF capacitor. If it's an
electrolytic capacitor, then the leakage current noise will will destroy
the stability. If it's a ceramic capacitor, then its piezoelectric
properties will couple any acoustic noise and vibration into your
EFC voltage.

Best to ground the EFC voltage and then use a phase/frequency
stepper to shift the frequency of the BVA using a digital control
loop.-

I can only evaluate this using GNSS PPP - by
RTKLib in real time or NRCAN for example and / or CGGTTS files.

I have also available for these measurements a frequency comb from menlo
systems. Can I use repetition rate adev to evaluate the BVA? (locking it in
a Cs beam and then in BVA + Cs beam)?

If the frequency comb is CEO stabilized (aka f-2f lock) and you can
stabilize its repetition rate using an optical cavity (10cm ULE is
already enough), then you can get better stability than your BVA
in the range up to 10s probably better than 100s, depending on your
setup. If the comb is free running, then the intrinsic instability
of the comb will be larger than the BVA.

We are working in cold atom clocks here also. A Cs fountain and another
kind of cold atom Cs clock. But now, we're in the construction phase. No
measurements being made.

Oh nice! Do you already have any publications on this?
I could only find [1] and [2].

BTW: If you want some known-good reference. The Canadians (IIRC the
NRC itself) sell caesium fountains for a reasonable price.

About getting the maser working again, do you have any experience with that
maser? Is the KVARZ CH1-75A.

I have never personally worked on a AHM myself. I do know their
working principle and how the electronics is supposed to look.
Unfortunately, I don't know anyone at Kvarz, only at the former
T4-Science.

		Attila Kinali

[1] "Progress in Brazilian Cesium atomic fountain-BrCsF",
by Rodriguez, Bagnato, Bueno et al, 2016
https://doi.org/10.1109/FCS.2016.7546818

[2] "Progress toward Brazilian cesium fountain second generation",
by Bueno, Rodriguez, Müller, et al. 2018
http://dx.doi.org/10.1088/1742-6596/975/1/012071

--
The driving force behind research is the question: "Why?"
There are things we don't understand and things we always
wonder about. And that's why we do research.
-- Kobayashi Makoto

A wonderful good afternoon, On Thu, 28 May 2026 10:37:58 -0300 Luiz Paulo Damaceno via time-nuts <time-nuts@lists.febo.com> wrote: > Thank you for the considerations. I've tunned the PLL for 0.00289Hz, today > i'm using a 1,1M ohm resistance and 50 uF capacitor. I can also reduce the > error voltage by changing the voltage in a potentiometer, just like a > "volume" control in audio systems. I expect to reduce a bit 0,25 times day > to day) to archive 1000s loop. A PLL using the EFC input of the BVA will not work well at these long time constants. About 1Hz loop bandwidth is the lowest that's reasonable, I would even draw the line at 10Hz. And only if you build an active filter using an low-noise opamp. Going lower will limit your oscillators stability by the noise on the EFC voltage. You have a 1MΩ resistor, which already produces quite a bit of noise voltage. And then you use a 50µF capacitor. If it's an electrolytic capacitor, then the leakage current noise will will destroy the stability. If it's a ceramic capacitor, then its piezoelectric properties will couple any acoustic noise and vibration into your EFC voltage. Best to ground the EFC voltage and then use a phase/frequency stepper to shift the frequency of the BVA using a digital control loop.- > I can only evaluate this using GNSS PPP - by > RTKLib in real time or NRCAN for example and / or CGGTTS files. > > I have also available for these measurements a frequency comb from menlo > systems. Can I use repetition rate adev to evaluate the BVA? (locking it in > a Cs beam and then in BVA + Cs beam)? If the frequency comb is CEO stabilized (aka f-2f lock) and you can stabilize its repetition rate using an optical cavity (10cm ULE is already enough), then you can get better stability than your BVA in the range up to 10s probably better than 100s, depending on your setup. If the comb is free running, then the intrinsic instability of the comb will be larger than the BVA. > We are working in cold atom clocks here also. A Cs fountain and another > kind of cold atom Cs clock. But now, we're in the construction phase. No > measurements being made. Oh nice! Do you already have any publications on this? I could only find [1] and [2]. BTW: If you want some known-good reference. The Canadians (IIRC the NRC itself) sell caesium fountains for a reasonable price. > About getting the maser working again, do you have any experience with that > maser? Is the KVARZ CH1-75A. I have never personally worked on a AHM myself. I do know their working principle and how the electronics is supposed to look. Unfortunately, I don't know anyone at Kvarz, only at the former T4-Science. Attila Kinali [1] "Progress in Brazilian Cesium atomic fountain-BrCsF", by Rodriguez, Bagnato, Bueno et al, 2016 https://doi.org/10.1109/FCS.2016.7546818 [2] "Progress toward Brazilian cesium fountain second generation", by Bueno, Rodriguez, Müller, et al. 2018 http://dx.doi.org/10.1088/1742-6596/975/1/012071 -- The driving force behind research is the question: "Why?" There are things we don't understand and things we always wonder about. And that's why we do research. -- Kobayashi Makoto